NGC 4599 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Virgo. It was discovered by the astronomer William Herschel in 1784. The galaxy is notable for its bright central bar structure and well-defined spiral arms, which are characteristic features of barred spiral galaxies. This galaxy has an apparent magnitude of about 12.5, making it faintly visible through small telescopes. NGC 4599 is part of the Virgo Cluster, a group of galaxies that includes many other notable members, contributing to our understanding of galaxy formation and evolution.